Omnigeneity: Difference between revisions
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* [[Stellarator]] | * [[Stellarator]] | ||
* [[Quasisymmetry]] | * [[Quasisymmetry]] | ||
* [[Piecewise_omnigeinity]] | |||
== References == | == References == | ||
<references /> | <references /> | ||
Latest revision as of 11:55, 9 February 2026
Omnigeneity (or omnigenity) is a property of the vacuum magnetic field such that the mean radial collisionless guiding center magnetic drift is zero. Thus, in a perfectly omnigenous field, all collisionless trajectories are confined. [1] [2]
See also
References
- ↑ D.A. Garren and A.H. Boozer, Existence of quasihelically symmetric stellarators, Phys. Fluids B 3 (1991) 2822
- ↑ M. Landreman and P.J. Catto, Omnigenity as generalized quasisymmetry, Phys. Plasmas 19 (2012) 056103